Stereo Pairs 
An explanation of stereo pairs and their use (PDF)  

Planned stereo pairs have suitable stereo convergence angles and illumination by design. In addition to planned stereo pairs, the Pairendipity software can identify overlapping HiRISE images that are serendipitously suitable for stereo processing and find stereo pairs within the CTX dataset.

Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below. Since this list is based on produced stereo anaglyphs it also contains a few serendipitous pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed in the “Pairendipity Stereo” link, while CTX stereo pairs are listed in “Pairendipity CTX Stereo”.

Images taken close together in time minimize illumination and frost differences and are especially useful (see the Delta-Days column in the Pairendipity files or difference the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.

Lava Flow in Kasei Valles:   ESP_066848_1985   ESP_067323_1985   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
18.53

285.

-2.5

-15.5

54.3

50.0

Crater Fill Material:   ESP_066791_2045   ESP_067411_2045   (Interval in Earth days: 49)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.10

40.8

-4.5

19.86

58.8

50.1

Subtle Scarp in South Polar Layered Deposits:   ESP_066852_0920   ESP_067078_0920   (Interval in Earth days: 18)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-87.8

221.

18.9

8.195

69.2

73.9

Scarp Fronted Deposit in South Gunjur Crater:   ESP_066774_1795   ESP_067526_1795   (Interval in Earth days: 59)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-0.32

146.

8.48

17.64

43.5

38.5

Slope Streaks in Arabia Terra:   ESP_066514_2050   ESP_074889_2050   (Interval in Earth days: 652)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
24.59

40.0

-5.9

9.124

62.5

64.9

Relatively Pristine 7-Kilometer Crater with Gullies:   ESP_066597_1435   ESP_066465_1435   (Interval in Earth days: 10)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-36.3

302.

1.02

24.41

39.4

37.9

Craters with Steep Slopes:   ESP_066516_1445   ESP_084570_1445   (Interval in Earth days: 1407)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.1

352.

1.33

7.927

39.4

36.6

Central Deposit and Possible Exit Breach:   ESP_066805_1440   ESP_067557_1440   (Interval in Earth days: 59)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.7

25.9

1.63

11.85

39.1

44.5

Layered Deposits within Depression in Osuga Valles:   ESP_066583_1650   ESP_065897_1650   (Interval in Earth days: 53)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.8

322.

-10.

10.02

41.2

46.6

Tilted Strata in Central Structure of Martin Crater:   ESP_066848_1585   ESP_067798_1585   (Interval in Earth days: 74)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-21.4

290.

-0.1

-9.63

37.8

43.4


  


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